On the reconstruction of the surface structure of the spotted stars

dc.contributor.author	Kolbin A.
dc.contributor.author	Shimansky V.
dc.contributor.author	Sakhibullin N.
dc.date.accessioned	2018-09-18T20:15:27Z
dc.date.available	2018-09-18T20:15:27Z
dc.date.issued	2013
dc.identifier.issn	1063-7729
dc.identifier.uri	https://dspace.kpfu.ru/xmlui/handle/net/138036
dc.description.abstract	We have developed and tested a light-curve inversion technique for photometric mapping of spotted stars. The surface of a spotted star is partitioned into small area elements, over which a search is carried out for the intensity distribution providing the best agreement between the observed and model light curves within a specified uncertainty. We have tested mapping techniques based on the use of both a single light curve and several light curves obtained in different photometric bands. Surface reconstruction artifacts due to the ill-posed nature of the problem have been identified. © 2013 Pleiades Publishing, Ltd.
dc.relation.ispartofseries	Astronomy Reports
dc.title	On the reconstruction of the surface structure of the spotted stars
dc.type	Article
dc.relation.ispartofseries-issue	7
dc.relation.ispartofseries-volume	57
dc.collection	Публикации сотрудников КФУ
dc.relation.startpage	548
dc.source.id	SCOPUS10637729-2013-57-7-SID84880157529

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Публикации сотрудников КФУ Scopus [24551]
Коллекция содержит публикации сотрудников Казанского федерального (до 2010 года Казанского государственного) университета, проиндексированные в БД Scopus, начиная с 1970г.